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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <front>
    <journal-meta><journal-id journal-id-type="publisher">GMD</journal-id><journal-title-group>
    <journal-title>Geoscientific Model Development</journal-title>
    <abbrev-journal-title abbrev-type="publisher">GMD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Geosci. Model Dev.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1991-9603</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/gmd-12-3119-2019</article-id><title-group><article-title>Comparison of different sequential assimilation algorithms for
satellite-derived leaf area index using the Data Assimilation Research
Testbed (version Lanai)</article-title><alt-title>Comparing algorithms for LAI assimilation</alt-title>
      </title-group><?xmltex \runningtitle{Comparing algorithms for LAI assimilation}?><?xmltex \runningauthor{X.-L. Ling et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Ling</surname><given-names>Xiao-Lu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Fu</surname><given-names>Cong-Bin</given-names></name>
          <email>fcb@nju.edu.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff3">
          <name><surname>Yang</surname><given-names>Zong-Liang</given-names></name>
          <email>liang@jsg.utexas.edu</email>
        <ext-link>https://orcid.org/0000-0003-3030-0330</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Guo</surname><given-names>Wei-Dong</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0299-6393</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institute for Climate and Global Change Research and School of
Atmospheric Sciences, Nanjing University, <?xmltex \hack{\break}?> Nanjing 210023, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Joint International Research Laboratory of Atmospheric and Earth
System Sciences of Ministry of Education,<?xmltex \hack{\break}?> Nanjing 210023, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Geological Sciences, John A. and Katherine G. Jackson School of Geosciences, <?xmltex \hack{\break}?>University of Texas at Austin, Austin, TX 78705, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Cong-Bin Fu (fcb@nju.edu.cn) and Zong-Liang Yang (liang@jsg.utexas.edu)</corresp></author-notes><pub-date><day>22</day><month>July</month><year>2019</year></pub-date>
      
      <volume>12</volume>
      <issue>7</issue>
      <fpage>3119</fpage><lpage>3133</lpage>
      <history>
        <date date-type="received"><day>18</day><month>September</month><year>2018</year></date>
           <date date-type="rev-request"><day>3</day><month>January</month><year>2019</year></date>
           <date date-type="rev-recd"><day>12</day><month>June</month><year>2019</year></date>
           <date date-type="accepted"><day>17</day><month>June</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 Xiao-Lu Ling et al.</copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019.html">This article is available from https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019.html</self-uri><self-uri xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019.pdf">The full text article is available as a PDF file from https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e129">The leaf area index (LAI) is a crucial parameter for
understanding the exchanges of mass and energy between terrestrial
ecosystems and the atmosphere. In this study, the Data Assimilation Research
Testbed (DART) has been successfully coupled to the Community Land Model
with explicit carbon and nitrogen components (CLM4CN) by assimilating Global
Land Surface Satellite (GLASS) LAI data. Within this framework, four
sequential assimilation algorithms, including the kernel filter (KF), the
ensemble Kalman filter (EnKF), the ensemble adjust Kalman filter (EAKF), and
the particle filter (PF), are thoroughly analyzed and compared. The results
show that assimilating GLASS LAI into the CLM4CN is an effective method for
improving model performance. In detail, the assimilation accuracies of the
EnKF and EAKF algorithms are better than those of the KF and PF algorithm.
From the perspective of the average and RMSD, the PF algorithm performs worse
than the EAKF and EnKF algorithms because of the gradually reduced
acceptance of observations with assimilation steps. In other words, the
contribution of the observations to the posterior probability during the
assimilation process is reduced. The EAKF algorithm is the best method
because the matrix is adjusted at each time step during the assimilation
procedure. If all the observations are accepted, the analyzed LAI seem to be
better than that when some observations are rejected, especially in
low-latitude regions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\newpage}?>
<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e143">Land surface processes play an important role in the earth system because
all the physical, biochemical, and ecological processes occurring in the
soil, vegetation, and hydrosphere influence the mass and energy exchanges
during land–atmosphere interactions (Bonan, 1995; Pitman, 2003; Pitman et
al., 2009, 2012). The leaf area index (LAI) is a key biophysical parameter
of vegetation in land surface models (LSMs) and influences their simulation
performance. Therefore, high-quality, spatially and temporally continuous
LAI inputs are extremely important (Bonan et al., 1992; Li et al., 2015).</p>
      <p id="d1e146">Real-time monitoring of LAI on a large scale is a worldwide problem. The
lack of spatial representativeness caused by the sparse distribution of
conventional observations makes it difficult to achieve a global
observational LAI dataset. Remote sensing can provide global data with high
spatial and temporal resolutions, but the inversion accuracy is associated
with different plant functional types (PFTs) and vegetation fractions.
Furthermore, although advanced land surface models (LSMs, e.g., the
Community Land Model version 4, CLM4) can predict LAI variation, the model
performance is greatly affected by the model structure, meteorological forcing, and initial and boundary conditions of the input (Dai et al., 2003; Luo et
al., 2003; Levis et al., 2004). Data assimilation (DA), through optimally
combining both dynamical and<?pagebreak page3120?> physical mechanisms with real-time
observations, can effectively reduce the estimation uncertainties caused by
spatially and temporally sparse observations and poor observed data accuracy
(Kalnay, 2003).</p>
      <p id="d1e149">As a link between observations and dynamic model states, mathematical
algorithms play an important role in calculating the increments and
adjusting the state vector during assimilation (Kalnay et al., 2007). The
two basic data assimilation algorithms are the variational DA based on
optimal control theory and sequential algorithms based on the Kalman filter (Dimet and Talagrand, 1986; Gordon et al., 1993; Bannister,
2017; Vetra-Carvalho et al., 2018). Because the Kalman filter algorithm is based on the
linear model error assumption, many new sequential algorithms have been
proposed. For example, the extended Kalman filter (EKF) was developed to
meet the need for a nonlinear observation operator, but the tangent operator
needs to be developed (Kalnay, 2003). Based on the Monte Carlo method and
focused on the nonlinear operator, the ensemble Kalman filter (EnKF) was
developed (Evensen, 1994) and was first used in the study of atmospheric
science (Houtekamer and Mitchell, 1998). Since then, the EnKF has been
widely applied for the assimilation of ocean, land surface, and atmospheric
data (Houtekamer et al., 2005; Evensen, 2007). In recent years, the
Monte Carlo methods have been proposed to allow the assimilation of
information from sources that have non-Gaussian errors.</p>
      <p id="d1e152">Many previous studies focusing on the comparison of variational and
sequential algorithms have been conducted to determine the optimal
assimilation method (Han and Li, 2008). Wu et al. (2011) systematically
compared the EnKF, 3DVAR, and 4DVAR algorithms and found that the EnKF algorithm
was better than the 3DVAR method and the same as the 4DVAR method. For this
reason, the application of the EnKF algorithm has been expanded quickly, and
many other forms of the EnKF method have been developed, such as the dual
EnKF (Li et al., 2014), ensemble square root filter (EnSRF) (Whitaker and
Hamill, 2002), and ensemble adjust Kalman filter (EAKF, Anderson, 2001). At
the same time, combinations of variational algorithms and sequential
algorithms have also been developed. For example, the maximum likelihood
ensemble filter (MLEF, Zupanski, 2005), the combination of 3DVAR and PF
algorithms (Leng and Song, 2013), and the hybrid variational-ensemble data
assimilation methods, i.e., the 4DEnKF (Hunt et al., 2004; Fertig et al.,
2007; Zhang et al., 2009) and the DrEnKF (Wan et al., 2009), have been
developed at NCEP and applied to improve model predictions (Whitaker et al., 2008).</p>
      <p id="d1e156">A complete Land Data Assimilation System (LDAS) is mainly composed of
forcing datasets, initial and boundary datasets, parameterization sets,
dynamical models as physical constraints, assimilation algorithms,
observational data, and target output. In recent decades, studies of land
data assimilation have become very active, although this topic was proposed
later than the assimilation of atmospheric observations (Lahoz and De
Lannoy, 2014). Land data assimilation can implement both in situ
observations and remotely sensed data like satellite observation of soil
moisture, snow water equivalent (SWE), land surface temperature, and so on to
constrain the physical parametrization and initialization of land surface
state. (Liu et al., 2008; Reichle et al., 2014; Zhang et al., 2014; Zhao et
al., 2016; Zhao and Yang, 2018). The widely acknowledged LDASs include the North LDAS
(NLDAS, Mitchell et al., 2004; NLDAS-2, Luo et al., 2003; Xia et al., 2012),
the Global LDAS (GLDAS, Rodell et al., 2004), the European LDAS (ELDAS,
Jacobs et al., 2008), the West China LDAS (WCLDAS, Huang and Li, 2004), and
the Canadian LDAS (CaLDAS, Carrera et al., 2015).</p>
      <p id="d1e159">Recent studies focusing on assimilation in terrestrial systems have tended
to add multiple phenological observations to constrain and predict biome
variables and further improve model performance (Knyazikhin et al., 1998;
Xiao et al., 2009; Viskari et al., 2015). Joint assimilation of surface
incident solar radiation, soil moisture, and vegetation dynamics (LAI) into
land surface models or crop models is of great importance since it can
improve the model results for national food policy and security assessments
(Sabater et al., 2008; Ines et al., 2013; Sawada et al., 2015; Jin et al.,
2018; Mokhtari et al., 2018). Furthermore, the ability to simulate river
discharge, land evapotranspiration, and gross primary production has been
improved in Europe (Barbu et al., 2011; Albergel et al., 2017). To date,
such studies have been conducted using a single sequential algorithm at a
single site or on regional scales (Montzka et al., 2012; Sawada, 2018).</p>
      <p id="d1e162">The Data Assimilation Research Testbed (DART) is an open-source community
facility and includes several different types of Kalman filter algorithms (Anderson et
al., 2009). It has been coupled to many high-order models and observations
for ocean, atmosphere, land surface, and chemical constituents. For example,
DART has been coupled with CLM4 or CLM4.5 to improve snow and soil moisture
estimations as well as land carbon processes (Zhang et al., 2014; Kwon et
al., 2016; Zhao et al., 2016; Fox et al., 2018; Zhao and Yang, 2018).
Utilizing the coupled DART–CLM4, the Global Land Surface Satellite LAI (GLASS
LAI) data are assimilated into the Community Land Model with carbon and
nitrogen components (CLM4CN) in the present study to explore the optimal
assimilation algorithm for model performance. The experimental design and
different assimilation algorithms are described in Sect. 2. Section 3
describes the optimal algorithm for LAI assimilation, and the proportion of
observations is discussed in Sect. 4. Conclusions and discussions are given
in Sect. 5.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methodology</title>
      <p id="d1e173">A complete LDAS is mainly composed of meteorological forcing, initial and boundary datasets,
parameterization sets, dynamical LSMs, assimilation algorithms,
observational data, and target output. LSMs play an important role<?pagebreak page3121?> in the
LDAS because they can add physical constraints to the control variables
during assimilation. In addition, the simulation ability of LSMs can
directly affect the output because they provide the associated uncertainty
for assimilation.</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>CLM4CN</title>
      <p id="d1e183">Developed by the National Center for Atmospheric Research (NCAR), the
Community Land Model (CLM) can simulate energy, momentum, and water exchanges
between the land surface and the overlying atmosphere at each computational
grid. The CLM is designed mainly for coupling with the atmospheric numerical
model and providing the surface albedo (direct and scattered light within
the visible and infrared bands), upward longwave radiation, sensible heat
flux, latent heat flux, water vapor flux, and east-to-west and
south-to-north surface stress needed by the atmospheric model. These
parameters are controlled by many ecological and hydrological processes. The
model can also simulate leaf phenology and physiological processes, as well
as water circulation through plant pores. Ecological differences between
vegetation types and thermal and hydrological differences between different
soil types are also considered. Each grid cell can be covered by several
different land use types. Each cell contains several land units, each land
unit contains a different number of soil and snow cylindrical blocks, and
each cylindrical block may contain several types of vegetation functions.
The CLM employs 10 soil layers to resolve soil moisture and temperature
dynamics and uses PFTs to represent subgrid vegetation heterogeneity (Oleson
et al., 2010).</p>
      <p id="d1e186">There are two ways to update LAI in CLM4. The LAI is treated as a diagnostic
variable that is linearly interpolated from a 30-year averaged satellite
dataset, and there is no annual LAI variation for CLM4 with satellite
phenology (CLM4SP) (Lawrence and Chase, 2007). For CLM4CN, the prognostic
LAI is calculated by the leaf carbon pool and an assumed vertical gradient
of specific leaf area (SLA) (Thornton and Zimmermann, 2007). Carbon and
nitrogen are obtained by plant storage pools in one growing season and then
retained and distributed in the subsequent year. All carbon and nitrogen
state variables in vegetation, litter, and soil organic matter (SOM) are
prognostic based on the prescribed vegetation phenology. The CLM4CN offline
mode with prescribed meteorological forcing is used in this study.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>DART (the Lanai version)</title>
      <p id="d1e197">DART is developed and maintained by the Data Assimilation Research Section
(DAReS) at NCAR. The purpose of DART is to provide a flexible tool for data
assimilation (DA), and it has been coupled with many high-order models. As
a software environment, DART makes it easy to explore a variety of data
assimilation methods and observations with different numerical models. The
DART system includes several different types of sequential algorithms, which
are selected at runtime by a namelist setting. The Lanai version of DART,
which supports many existing models including the CESM climate component,
the MPAS (Model for Prediction Across Scales) models, and the NOAH land model, is used in this study. Released in December 2013, the Lanai version of
DART can process many new observation types and sources and include new
diagnostic routines as well as new utilities. Detailed settings for DART can
be found at <uri>https://www.image.ucar.edu/DAReS/DART/</uri> (last access: 1 July 2019).</p>
      <p id="d1e203">Currently, the coupled DART–CLM4 model has produced many reanalysis data for
snow and soil moisture. It has been found that snow DA can improve
temperature predictions, especially over the Tibetan Plateau, implying great
implications for future land DA and seasonal climate prediction studies (Lin
et al., 2016). Furthermore, the coupled DART–CLM framework would be employed
to assimilate other variables, such as LAI, from various satellite sources
and ground observations (i.e., truly multimission, multiplatform,
multisensor, multisource, and multiscale). Ultimately, this would allow
earth system models to be constrained by all types of observations to
improve model performance for seasonal and decadal prediction skills.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Sequential assimilation algorithms</title>
      <p id="d1e214">According to Anderson (2001), Eq. (1) is used to express how new
sets of observations modify the prior joint state conditional probability
distribution obtained from predictions based on previous observation sets.
            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M1" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{9.5}{9.5}\selectfont$\displaystyle}?><mml:mtext mathvariant="bold">p</mml:mtext><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub><mml:mo>|</mml:mo><mml:msub><mml:mi mathvariant="bold">Y</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mtext mathvariant="bold">p</mml:mtext><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="bold">y</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow><mml:mi>o</mml:mi></mml:msubsup><mml:mo>|</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mtext mathvariant="bold">p</mml:mtext><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold">z</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub><mml:mo>|</mml:mo><mml:msub><mml:mtext mathvariant="bold">Y</mml:mtext><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi mathvariant="bold">p</mml:mi><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="bold">y</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup><mml:mo>|</mml:mo><mml:msub><mml:mi mathvariant="bold">Y</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>,</mml:mo><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
          in which <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Y</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is defined as the superset of all observation subsets,
<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">y</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is the <inline-formula><mml:math id="M4" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>th subset of observations
at time <inline-formula><mml:math id="M5" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the joint state–observation vector for a given <inline-formula><mml:math id="M7" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M8" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>.
In ensemble applications, generally there is no need to compute the
denominator of Eq. (1). Four algorithms for approximating the product in the
numerator of Eq. (1) are presented below, and detailed information can be found
in Anderson (2001).</p>
<sec id="Ch1.S2.SS3.SSS1">
  <label>2.3.1</label><title>Kernel filter (KF)</title>
      <p id="d1e443">The kernel filter (KF) mechanism, first proposed by Lindgren et al. (1993) and
further developed by Anderson and Anderson (1999), has been incorporated
into DART and can be extended to the joint state space. A detailed
calculation process can be found in Anderson (2001). The KF is
potentially general, because the values and expected values of the mean and
covariance and higher-order moments of the resulting ensemble are functions
of high-order moments of the prior distribution. However, when applied to
large models, computational efficiency will be an issue for the application
of the algorithm.</p>
</sec>
<?pagebreak page3122?><sec id="Ch1.S2.SS3.SSS2">
  <label>2.3.2</label><title>Ensemble Kalman filter (EnKF)</title>
      <p id="d1e454">The Kalman filter (Kalman, 1960)
algorithm has not been widely used because of computing limitations
and the linear model error assumption. The EnKF was proposed based on a
Monte Carlo approximation, for which the background error covariance is
approximated using an ensemble of forecasts (Evensen, 1994). The EnKF
algorithm can be utilized for nonlinear systems and can also reduce the
computing requirement of DA (Burgers et al., 1998; Evensen, 2003, 2007).</p>
      <p id="d1e457">The EnKF procedure is divided into two stages: prediction and analysis. (1) In the prediction stage, the ensemble forecast field is generated from the
ensemble initial condition, and the error covariance matrix of the ensemble
forecast is calculated. (2) In the analysis stage, the simulation of each
member of the ensemble is updated using the covariance matrix of the observation vector error and state vector error. The traditional EnKF, an ensemble of Kalman filters with each member using a different sample estimate of the
prior mean and observations, is used in this study (Houtekamer and
Mitchell, 1998).</p>
</sec>
<sec id="Ch1.S2.SS3.SSS3">
  <label>2.3.3</label><title>Ensemble adjust Kalman filter (EAKF)</title>
      <p id="d1e468">Although the forms of expression are different, the proposed EnSRF (Whitaker
and Hamill, 2002) and EAKF (Anderson, 2001) are the same algorithm.</p>
      <p id="d1e471">The difference between the EAKF and the traditional EnKF lies in the
adjustment of the gain matrix to avoid filtering the divergence problem by
increasing the premise of the analysis error covariance (Anderson, 2003,
2007; Wang et al., 2007). In the EAKF algorithm, ensemble observation
members are calculated by the observation operator, and the increment of
each observation member is calculated as <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e487">The increment <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>X</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> for each ensemble sample of each
state variable in terms of <inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> can then be calculated as
follows:
              <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M12" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>X</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi>j</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup></mml:mrow><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi>j</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where <inline-formula><mml:math id="M13" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> indicates the ensemble member, <inline-formula><mml:math id="M14" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> is the state vector member, <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi>j</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is the prior covariance of the state vector and observation, and
<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is the prior variance of observation.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS4">
  <label>2.3.4</label><title>Particle filter (PF)</title>
      <p id="d1e635">The particle filter (PF) is also a sequential Monte Carlo method, which is
based on the Bayesian sequential importance sampling method (SIS). The PF
algorithm finds a set of random samples in the state space to approximate
the probability density function and then replaces the integral operation
with the sample mean to obtain the process of minimum variance distribution
of the state (Moradkhani et al., 2005). The procedure of the PF algorithm
can also be divided into two frameworks: forecast and analysis.</p>
      <p id="d1e638">If there are enough observations, the posterior density at <inline-formula><mml:math id="M17" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> can be
approximated as
              <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M18" display="block"><mml:mrow><mml:mi>p</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>k</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msubsup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">|</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>Y</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>≈</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msub><mml:mi>w</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub><mml:mi mathvariant="italic">δ</mml:mi><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>k</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow><mml:mi mathvariant="normal">a</mml:mi></mml:msubsup><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

              <disp-formula id="Ch1.Ex1"><mml:math id="M19" display="block"><mml:mrow><mml:mi mathvariant="normal">where</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="italic">δ</mml:mi><mml:mfenced open="(" close=")"><mml:mo>∗</mml:mo></mml:mfenced><mml:mi mathvariant="normal">is</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">the</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">Dirac</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">function</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">and</mml:mi><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msub><mml:mi>w</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            in which <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>k</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msubsup><mml:mi mathvariant="normal">|</mml:mi><mml:msub><mml:mi>Y</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> is the posterior probability
distribution, <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow><mml:mi mathvariant="normal">a</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is the particle
element, <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the weight of each
particle, and <inline-formula><mml:math id="M23" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> is the number of particles. Unlike the EnKF algorithm, the PF
method takes into account the weights of different particles and can be
better applied to nonlinear systems. However, in association with the DA,
there are a limited number of particles with large weights, and too many
computing resources are distributed to particles with weights of
approximately 0. This situation is called particle degradation (Doucet et
al., 2000). Effective methods to solve this issue include resampling or
selecting more reasonable importance functions.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Datasets</title>
<sec id="Ch1.S2.SS4.SSS1">
  <label>2.4.1</label><title>Ensemble meteorological forcing and initial conditions</title>
      <p id="d1e880">The ensemble initial conditions and background error (Hu et al., 2014) are
produced from ensemble analysis products generated by running DART and the
Community Atmosphere Model (CAM4) (Raeder et al., 2012). DART–CAM4 produced
80 atmospheric forcing datasets with 6 h time intervals for the period of
1998–2010. These ensemble meteorological data have been widely employed in
DA for ocean, snow, soil moisture, and many other related studies
(Danabasoglu et al., 2012). By considering computational cost and filter
performance, 40 members among the ensemble forcing datasets are chosen to
drive the CLM4CN.</p>
      <p id="d1e883">To achieve a steady state solution for all state variables, the CLM4CN was
run for 4000 years using Qian's forcing (Qian et al., 2006) at the resolution
of 1.9<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude by 2.5<inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude (Shi et al., 2013).
The CLM4CN was then forced by the ensemble mean of selected 40 members of
DART–CAM datasets for 1000 years. In the last step, the ensemble simulation
during the time period from 1998 to 2001 was treated as a spin-up process, and
40 ensemble initial conditions were obtained. Aiming at a global scale and
considering the computational cost, only 1-year assimilation and ensemble
simulation were conducted. Our goal is to first find out the best
experiment and then conduct long-term simulation or assimilation in the future.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e907">Experimental design for LAI assimilation using DART–CLM4CN.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Assimilated</oasis:entry>
         <oasis:entry colname="col3">Updated</oasis:entry>
         <oasis:entry colname="col4">Assimilation</oasis:entry>
         <oasis:entry colname="col5">Accept all</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Experiment</oasis:entry>
         <oasis:entry colname="col2">variables</oasis:entry>
         <oasis:entry colname="col3">variables</oasis:entry>
         <oasis:entry colname="col4">algorithm</oasis:entry>
         <oasis:entry colname="col5">observation</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Algorithms</oasis:entry>
         <oasis:entry colname="col2">GLASS LAI</oasis:entry>
         <oasis:entry colname="col3">LAI, Leaf C, Leaf N</oasis:entry>
         <oasis:entry colname="col4">EAKF, EnKF, KF, PF</oasis:entry>
         <oasis:entry colname="col5">No</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Algorithms without</oasis:entry>
         <oasis:entry colname="col2">GLASS LAI</oasis:entry>
         <oasis:entry colname="col3">LAI, Leaf C, Leaf N</oasis:entry>
         <oasis:entry colname="col4">EAKF</oasis:entry>
         <oasis:entry colname="col5">Yes</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">observation rejection</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e1020">Spatial distributions of global LAI values in 2002 for <bold>(a)</bold> GEOV2
LAI in July, <bold>(b)</bold> ensemble mean of simulations in July, <bold>(c)</bold> GEOV2 LAI in
November, and <bold>(d)</bold> ensemble mean of simulations in November.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f01.png"/>

          </fig>

</sec>
<sec id="Ch1.S2.SS4.SSS2">
  <label>2.4.2</label><title>LAI datasets</title>
      <p id="d1e1049">The Global Land Surface Satellite (GLASS) LAI dataset is used in this study
as observations for assimilation (Zhao et<?pagebreak page3123?> al., 2013). Since the ensemble
simulation or assimilation is run at the resolution of 0.9<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
latitude by 1.25<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude, the original spatial resolution of
0.05<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> of the GLASS LAI is upscaled to the same resolution.</p>
      <p id="d1e1079">An independent LAI dataset from the Copernicus Global Land Service (CGLS)
with version 2 (GEOV2 LAI) was utilized to validate the assimilation result.
The GEOV2 LAI is derived from the vegetation instruments on Satellite Pour
I'Observation de la Terre (SPOT-VGT) and on board the PROBA satellite (PROBA-V
satellites) (Verger et al., 2014). The resolution of GEOV2 LAI is 1 km,
which is also upscaled to the grid level to evaluate the analysis of LAI and
assimilation effect.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e1084">Differences between global LAI from assimilation experiments with
the methods of <bold>(a)</bold> EAKF, <bold>(b)</bold> EnKF, <bold>(c)</bold> KF, and <bold>(d)</bold> PF and GEOV2 LAI in July 2002.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f02.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e1108">Same as Fig. 2 but for RMSE of ensemble members.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f03.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Experimental design</title>
      <p id="d1e1126">To determine the optimal assimilation algorithm, five experiments
corresponding to the KF, EnKF, EAKF, and PF methods are designed and shown
in Table 1, in which the “Algorithms” experiments would reject some
observations under certain conditions using the KF, EnKF, EAKF, and PF
algorithms. The expected value of the difference between the prior mean and
observation is <inline-formula><mml:math id="M29" display="inline"><mml:msqrt><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">prior</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">obs</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:msqrt></mml:math></inline-formula>, in which <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">prior</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are
standard deviations of the prior probability density function (PDF)
and observation PDF respectively. DART
will reject the observation if the bias of the prior mean and observations
is larger than 3 times the expected value. The “Algorithms without
observation rejection” experiments would accept all the observed LAI.
During assimilation, CLM stops and writes restart and history files at a
frequency of 8 d. If there are available observational GLASS LAI data,
they are assimilated into the CLM4CN. DART extracts the state vector; the
increments are calculated by filtering at each time step; and the LAI, leaf
carbon (Leaf C), and leaf nitrogen (Leaf N) are updated. The adjusted DART
state vector is resent to the CLM restart files as a new initial condition
for the next time step. All the simulation and assimilation are conducted at
the spatial resolution of 0.9<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude by 1.25<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
longitude. The ensemble assimilation is conducted point wise, indicating that
spatial covariances are not considered.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e1194">RMSDs of ensemble means of simulation and assimilation versus GEOV2
LAI for <bold>(a)</bold> global, <bold>(b)</bold> boreal (45–65<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), <bold>(c)</bold> northern temperate (23–45<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), <bold>(d)</bold> northern equatorial (0–23<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), <bold>(e)</bold> southern equatorial (0–23<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S), and <bold>(f)</bold> southern temperate
(23–90<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f04.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e1269">Globally or regionally averaged RMSDs for the
simulation and assimilation results and GEOV2 LAI.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f05.png"/>

        </fig>

</sec>
</sec>
<?pagebreak page3124?><sec id="Ch1.S3">
  <label>3</label><title>The optimal algorithm for DART–CLM4CN</title>
      <p id="d1e1287">The spatial distributions of global LAI in 2002 for (a) GEOV2 LAI in July,
(b) ensemble mean of simulations in July, (c) GEOV2 LAI in November, and
(d) ensemble mean of simulations in November are shown in Fig. 1. The
observations in Fig. 1 are from the upscaled GEOV2 LAI dataset with a
spatial resolution of 0.9<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude by 1.25<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude. There are two
latitudinal belts of high LAI values located in the tropics and at
50–65<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in July. These two regions are mainly dominated by
evergreen broadleaf forests and boreal forests, respectively. There are three
high-LAI regions located in the tropics: the Amazon, central Africa, and
some islands in Southeast Asia. Because of the presence of deserts, plateaus,
and bare ground, the LAI is low in northern Africa, western North America,
western Australia, southern Africa,<?pagebreak page3125?> and southern South America, where shrubs
and/or grass are dominant. Globally, the CLM4CN can simulate the LAI
distribution characteristics, except that it systematically overestimates
LAI, especially at low latitudes and boreal forest regions, with the largest
bias of 5 m<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. The global LAI is lower in November than in July.
The LAI values in the high latitudes of the Northern Hemisphere are higher
in July than in November because November is not the growing season for most
of the vegetation in the Northern Hemisphere.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e1340">The histograms of innovation and residuals of LAI globally and for
all subregions during July 2002. <bold>(a–d)</bold> Global; <bold>(e–h)</bold> boreal; <bold>(i–l)</bold> northern
temperate; <bold>(m–p)</bold> northern equatorial; <bold>(q–t)</bold> southern equatorial; <bold>(u–x)</bold> southern temperate.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f06.jpg"/>

      </fig>

      <p id="d1e1368">The differences between the methods of (a) EAKF, (b) EnKF, (c) KF, and
(d) PF and GEOV2 LAI are displayed in Fig. 2. Globally, the differences
between assimilation with the four methods and GEOV2 LAI are larger in
lower-latitude regions, indicating that assimilation also overestimates the
LAI value in these regions. The biases of assimilation and observation
reduce to 2 m<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the low-latitude regions compared with the
biases of simulation and observation in Fig. 1, where they are dominated by BET tropical and mixed forest types. The LAI values from the assimilation
experiment are always 1 m<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> higher in the middle- and
high-latitude regions, especially in western North America, northwestern
China, and western Australia, where open shrublands and grasslands are
dominant. Assimilation always underestimates the LAI values in eastern
North America, northeastern China, and the 50–65<inline-formula><mml:math id="M48" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N latitude
regions of Eurasia, where they are dominated by NET boreal forests and mixed
forest types. The assimilation with the EAKF and EnKF algorithms displays a
lower bias than the KF and PF algorithms compared to GEOV2 LAI, especially
in the northern and eastern Amazon, central Africa, southern Eurasia, and
Southeast Asia. Notably, the correction of overestimated LAI is
significantly better than that of underestimated LAI, which is mainly
attributed to the high dispersion of LAI in those regions. In other words,
high dispersion is beneficial to assimilation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e1425">The proportion of accepted LAI observations for the four
algorithms in the zonal regions.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f07.png"/>

      </fig>

      <p id="d1e1434">The results also indicate that the EAKF and EnKF assimilation algorithms are
better than the KF and PF algorithms in November (figures not shown). In
detail, the EAKF algorithm is better than the EnKF method in November,
especially in the Amazon, central Africa, and southern Eurasia. The biases
of assimilated LAI relative to the observed LAI are higher in November in
the 20–65<inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N region, which may be because vegetation during this
period in the Northern Hemisphere is not lush. In western Australia and
central<?pagebreak page3126?> Eurasia, the improvement of the underestimation in November is not
as significant as that in July, which indicates that the system has a
limited capability to simulate the vegetation process, especially for open
shrubland and grassland. From the perspective of the average and RMSE, the
PF algorithm performs worse than the EAKF and EnKF algorithms because of the
gradually reduced acceptance of observations with assimilation steps (will
discuss below). Note that the average and RMSE only make sense for the
ensemble Kalman filters. For the PF algorithm, the particle with the largest
weight (a posteriori maximum for the PDF) should be discussed separately.</p>
      <p id="d1e1446">The RMSEs of ensemble members are shown in Fig. 3 to provide hints where
the assimilation is the most efficient. The RMSEs of ensemble members for
the EAKF and EnKF algorithm are larger than those for the KF and PF
algorithms, indicating that the EAKF and EnKF are more effective. In July 2002, the RMSE of the ensemble estimates is the largest in lower-latitude regions, with particularly high values in central South America, central
Africa, and Southeast Asia. The regions with comparatively large ensemble
spreads are located in western North America and western Europe. The large
ensemble spreads areas are also transitional regions with different
vegetation types, indicating low capability of the models to simulate
complex vegetation types.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e1451">Differences between globally assimilated and GEOV2 LAIs for the
methods of EAKF in <bold>(a)</bold> July and <bold>(b)</bold> November.</p></caption>
        <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f08.png"/>

      </fig>

      <p id="d1e1466">The globally mean LAI and the LAI in five latitudinal bands were chosen for
analysis in this study. The five bands are boreal (45–65<inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N),
northern temperate (23–45<inline-formula><mml:math id="M51" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), northern equatorial
(0–23<inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), southern equatorial (0–23<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S), and southern
temperate (23–90<inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S). Figure 4 presents the root-mean-square
deviation (RMSDs) of the ensemble means of simulation and assimilation versus
GEOV2 LAI for (a) global, (b) boreal, (c) northern temperate, (d) northern
equatorial, (e) southern equatorial, and (f) southern temperate. Generally,
although they all feature similar variation pattern characteristics, the
RMSDs of all the assimilation datasets relative to the GEOV2 LAI are less
than those of the simulation, indicating that all four<?pagebreak page3127?> assimilation
algorithms can improve the LAI estimation. For boreal regions, there are two
maxima for the RMSD in May and September respectively, which is also the
period with abrupt variation for the LAI value. During the growing season, the
RMSDs of LAI reach relatively low values, especially for the regions in the
middle and high latitudes of the Northern Hemisphere and high latitudes of
the Southern Hemisphere. In the low-latitude region covered by evergreen or
deciduous broadleaf forests, the RMSD does not present an obvious annual
change. The EnKF algorithm performed best in the boreal region with the
smallest RMSD, while it did not perform as well in the northern temperate and northern
equatorial regions. The EAKF algorithm presented the lowest RMSD in the
southern equatorial and southern temperate regions, as well as global
regions. The assimilation is far less efficient in the boreal region than in
other areas, which is partly attributed to the consistently low initial RMSD
during nongrowing seasons and limited capability of the models for
simulating processes associated with boreal forest type.</p>
      <p id="d1e1515">Figure 5 shows the globally or regionally averaged RMSDs of
simulation and assimilation and GEOV2 LAI. The RMSDs of assimilation are lower
than those of simulation, implying that assimilating remotely sensed LAI
data into the CLM4CN is an effective method for improving the model
performance. The difference between simulation and all four algorithms in
the northern and southern equatorial regions is larger than in other
regions, indicating that the assimilation is more efficient there. The
global averaged RMSD for LAI from the EAKF experiment is lower than the
other three algorithms, except for the boreal regions, indicating the better
performance in assimilation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e1520">RMSDs of simulation experiments with and without rejection
(EAKF_reject and EAKF_noreject) and GEOV2 LAI
for the <bold>(a)</bold> globe, <bold>(b)</bold> boreal (45–65<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), <bold>(c)</bold> northern temperate
(23–45<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), <bold>(d)</bold> northern equatorial (0–23<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), <bold>(e)</bold> southern equatorial (0–23<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S), and <bold>(f)</bold> southern temperate
(23–90<inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S) regions.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/3119/2019/gmd-12-3119-2019-f09.png"/>

      </fig>

      <p id="d1e1593">The background and analysis
departures are calculated as (1) innovations, which
are the differences between the assimilated LAI and model background; and
(2) residuals, which are the differences between the assimilated LAI and
analysis (Barbu et al., 2011). It was concluded that the LDAS system is
working well based on the condition that the residuals are reduced compared
to the innovations (Albergel et al., 2017). Figure 6 shows the histograms of
innovation and residuals of LAI globally and for all subregions during July 2002. Generally, the distribution characteristics of both innovations and
residuals are similar for the algorithms of KF and PF, which means that
these two algorithms are not very efficient for LAI assimilation. The
distribution of residuals is more centered on 0 than that of the innovations
for the EAKF and EnKF algorithms, especially for the EAKF algorithm. The
innovations dominantly exhibit a large negative bias, indicating that the
model always highly overestimates LAI. The residuals can improve this
overestimation situation, especially for the EAKF algorithm. The analysis
departures for the EAKF<?pagebreak page3128?> algorithm are more centered on 0 than the EnKF
algorithm, especially in global, northern temperate, and southern temperate
regions.</p>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Effective observational proportion</title>
      <p id="d1e1605">The assimilation results depend not only on the algorithm but also on the
observations. This not only requires a sufficiently strong degree of
discretization for ensemble simulations but also requires the observational
variables to be sufficiently trustworthy. In this section, the proportion of
LAI observations that can be accepted for the four algorithms is discussed.
During assimilation, DART can calculate the number of nonassimilated
observations when the difference of prior mean and observations is larger
than 3 times the expected value. The proportion of accepted LAI
observations is defined as the number of accepted observations divided by
the number of total observations.</p>
      <p id="d1e1608">To explain the relationship between the assimilation algorithms and observation
rejection, Fig. 7 displays the proportion of accepted LAI observations for
the four algorithms in the zonal regions. In general, the EnKF and EAKF
methods accepted many more observational LAI observations than the PF and KF
methods. In the low-latitude regions, the proportion of accepted LAI
observations is approximately 75 %, which is lower than in the
high-latitude regions. This may be because the broadleaf forest in tropical
regions can grow unrestrictedly in the model, producing LAI values that are
much higher than the observations. At the very beginning of assimilation,
DART rejects the largest proportion of LAI observations in the southern
equatorial, northern equatorial, and northern temperate zones due to large
biases between the simulation and the observations. Over time, the rejection
proportion gradually decreases for the northern equatorial, southern
equatorial, and southern temperate regions. As ensemble-analyzed LAI values tend to be relatively fixed, the rejection proportion increases over regions with small
LAI amplitudes, such as the northern temperate and boreal region. From May
to September in the boreal region and from April to September in the
northern temperate region, the proportion of accepted LAI observations is much smaller
than in the other regions. These two periods with abrupt variation for the LAI
value are also when the model simulation presents an obvious discrete
characteristic. This experiment illustrates the utility of the spin-up
process for ensemble initial conditions. Furthermore, the KF and PF
algorithms gradually reduce the acceptance of observations as assimilation
progresses, which may partially explain their worse performance than the
EnKF and EAKF algorithms (see Fig. 5).</p>
      <p id="d1e1611">The differences between globally assimilated and GEOV2 LAI with the methods
of EAKF (with rejection) in (a) July and (b) November are shown in Fig. 8 to
illustrate the role of observation proportion. It can be concluded that when
accepting all the observations, the assimilation results seem to be better
than when some observations are rejected during assimilation. Large negative
biases occur in the Amazon, central Africa, southern Eurasia, and the boreal
region, where the LAI is overestimated in the model. Large positive biases
occur in southeastern China, western North America, western Australia, and
central South America in July, partly due to the influence of
topography. In November the positive biases are observed around the whole
middle- and high-latitude regions of the Northern Hemisphere, indicating the
overestimation for the LAI value in nongrowing seasons.</p>
      <p id="d1e1614">During assimilation, the assimilated observations (GLASS LAI) are always
treated as true values. The question thus becomes how do the true values
influence the assimilation results? Figure 9 shows the RMSDs of simulation
experiments with and without rejection (EAKF_reject and EAKF_noreject) and GEOV2 LAI over the (a) global, (b) boreal,
(c) northern temperate, (d) northern equatorial, (e) southern equatorial,
and (f) southern temperate regions. In the EAKF_reject
experimental design, if the observed LAI is 3 times larger than the bias
between the simulation and the observations, the observation would be
rejected by DART, while in the EAKF_noreject experiment all
observed LAIs are assimilated. Generally, RMSDs for both simulation and
assimilation present obvious annual variations. The RMSD of assimilation is
far less than that of the simulation, although their characteristic
variation patterns are similar. This<?pagebreak page3129?> demonstrates the effectiveness of
assimilation for improving model simulation. The RMSD relative to the
observations was highest for the simulation, followed by the
EAKF_reject experiment, and was lowest for the
EAKF_noreject experiment. During assimilation, when accepting
all the observations, the RMSD is smaller than when rejecting some
observations. Compared with the EAKF_reject experiment and other
algorithms in Fig. 5, the globally and regionally averaged RMSDs from the
EAKF_noreject experiment is much smaller, indicating the most
efficient performance.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions and discussion</title>
      <p id="d1e1625">The Community Land Model version 4 with prognostic carbon and nitrogen
components (CLM4CN) is coupled with the Data Assimilation Research Testbed
(DART) to determine the optimal assimilation algorithm for leaf area index
(LAI). The kernel filter (KF), ensemble Kalman filter (EnKF), ensemble
adjust Kalman filter (EAKF), and particle filter (PF) are discussed in this paper.</p>
      <p id="d1e1628">The results show that assimilating remotely sensed LAI into the CLM4CN is an
effective method for improving model performance. Globally speaking, the
EAKF and EnKF assimilation algorithms are better than the KF and PF
assimilation algorithms. The LAI obtained by the EAKF algorithm is more
continuous than that obtained by the EnKF algorithm and more consistent with
observations in central South American and central Africa, whereas the
deviation in the EnKF method can be from <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>  to 4 m<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Furthermore, the assimilation shows better performance in
the vegetation growing season. The lowest root-mean-square deviation
is associated with the EAKF algorithm, suggesting that the EAKF algorithm is
the best and has a robust performance.</p>
      <p id="d1e1662">The proportion of observations accepted by the land data assimilation system
is another topic of this research. The proportion of accepted LAI
observations is 10 %–20 % in the low latitudes, which is lower than in the high
latitudes because of large biases between the assimilation and the
observations. In contrast, low observation acceptance does not mean bad assimilation results, indicating that assimilation performance relies on not only observation factor but also the background error and ensemble model performance. When
all the observations are accepted, the RMSD of the results is smaller than
that when some observations are rejected.</p>
      <p id="d1e1665">The ensemble assimilation is conducted point wise without considering spatial
covariances, which will be<?pagebreak page3130?> considered in the future. Furthermore, more
evolved techniques are needed to counteract the degeneracy of the particle filter.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e1672">The Community Land Model version 4.0 with carbon and nitrogen components
(CLM4CN) is a part of the Community Earth System Model version 1.1.1
(CESM1.1.1) developed by the National Center for Atmospheric Research
(NCAR). The CESM code can be downloaded from
<uri>http://www.cesm.ucar.edu/index.html</uri> (last access: 18 June 2019; CESM, 2019). Developed and maintained by the Data
Assimilation Research Section (DAReS) at NCAR, Data Assimilation Research
Testbed (DART version lanai) can be downloaded from
<uri xlink:href="https://www.image.ucar.edu/DAReS/DART_classic/DART_Overview.html#explanation">https://www.image.ucar.edu/DAReS/DART_classic/DART_Overview.html\#explanation</uri> (last access: 1 July 2019; DART, 2019).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1684">All of the authors participated in the development of the paper's findings
and recommendations.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1690">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1696">Kevin Raeder
(raeder@ucar.edu) is thanked for providing the DART_CAM4 reanalysis as
ensemble meteorological forcing. Tim Hoar, Long Zhao, and Yongfei Zhang are
thanked for part of the coding and coupling with DART and CLM4CN. We thank Carlos Sierra and the anonymous reviewers for exceptionally thoughtful reviews and suggestions that greatly improved this paper.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e1701">This research has been jointly supported by the National Key Research and Development Program of China (grant nos. 2016YFA0600300 and 2017YFA0604300) and the Jiangsu Collaborative Innovation Center for Climate Change.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1707">This paper was edited by Carlos Sierra and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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<abstract-html><p>The leaf area index (LAI) is a crucial parameter for
understanding the exchanges of mass and energy between terrestrial
ecosystems and the atmosphere. In this study, the Data Assimilation Research
Testbed (DART) has been successfully coupled to the Community Land Model
with explicit carbon and nitrogen components (CLM4CN) by assimilating Global
Land Surface Satellite (GLASS) LAI data. Within this framework, four
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improving model performance. In detail, the assimilation accuracies of the
EnKF and EAKF algorithms are better than those of the KF and PF algorithm.
From the perspective of the average and RMSD, the PF algorithm performs worse
than the EAKF and EnKF algorithms because of the gradually reduced
acceptance of observations with assimilation steps. In other words, the
contribution of the observations to the posterior probability during the
assimilation process is reduced. The EAKF algorithm is the best method
because the matrix is adjusted at each time step during the assimilation
procedure. If all the observations are accepted, the analyzed LAI seem to be
better than that when some observations are rejected, especially in
low-latitude regions.</p></abstract-html>
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